The notion of quasisymmetry (QS) as a basis for magnetic confinement design has been promising for a few decades now. Initially, QS emerged as a requirement on the magnetic field so that the neoclassical behavior of the stellarator is equivalent to that of an axisymmetric tokamak.[1]}, [2]} This allowed for the design of 3D stellarators without suffering excessively from unfavorable confinement due to \(1/\nu \)  transport.[3]}
